activity
19932026
most citedThe Gravitational Million-Body Problem

557 citations · 5.2k across the 80 of their papers we have counts for

collaborators

81 papers

astro-ph.GA2026

Discrepancies between Chandrasekhar's theory of relaxation and -body simulations

Kerwann Tep, Douglas C. Heggie

Globular clusters are systems which are known to be particularly well described by two-body relaxation. In recent decades many studies have shown that Chandrasekhar's orbit-average…

astro-ph.GA2024★ 13 cited

Dynamics of star clusters with tangentially anisotropic velocity distribution

Václav Pavlík, Douglas C. Heggie, Anna Lisa Varri +1

Recent high-precision observations with HST and Gaia enabled new investigations of the internal kinematics of star clusters (SCs) and the dependence of kinematic properties on the…

astro-ph.GA2023

Punctuated chaos and the unpredictability of the Galactic center S-star orbital evolution

Simon Portegies Zwart, Tjarda Boekholt, Douglas Heggie

We investigate the chaotic behavior of the S-star cluster in the Galactic center using precise -body calculations, free from round-off or discretization errors. Our findings rev…

astro-ph.IM2023

Punctuated Chaos and Indeterminism in Self-gravitating Many-body Systems

Tjarda C. N. Boekholt, Simon F. Portegies Zwart, Douglas C. Heggie

Dynamical chaos is a fundamental manifestation of gravity in astrophysical, many-body systems. The spectrum of Lyapunov exponents quantifies the associated exponential response to…

astro-ph.GA2022★ 30 cited

The Effect of Stars on the Dark Matter Spike Around a Black Hole: A Tale of Two Treatments

Stuart L. Shapiro, Douglas C. Heggie

We revisit the role that gravitational scattering off stars plays in establishing the steady-state distribution of collisionless dark matter (DM) around a massive black hole (BH).…

astro-ph.GA2021★ 9 cited

The Kinematic Richness of Star Clusters - II. Stability of Spherical Anisotropic Models with Rotation

Philip G. Breen, Simon Rozier, Douglas C. Heggie +1

We study the bar instability in collisionless, rotating, anisotropic, stellar systems, using N-body simulations and also the matrix technique for calculation of modes with the pert…